MAVEN IUVS observation of the hot oxygen corona at Mars

E-ISSN： 1944-8007|42|21|9009-9014

ISSN： 0094-8276

Source： GEOPHYSICAL RESEARCH LETTERS, Vol.42, Iss.21, 2015-11, pp. : 9009-9014

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

A comparison of 3‐D model predictions of Mars' oxygen corona with early MAVEN IUVS observations

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9015-9022

John Wiley & Sons Inc

Access to resources Recommend Favorite

Three‐dimensional structure in the Mars H corona revealed by IUVS on MAVEN

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9001-9008

John Wiley & Sons Inc

Access to resources Recommend Favorite

Study of the Martian cold oxygen corona from the O I 130.4 nm by IUVS/MAVEN

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9031-9039

John Wiley & Sons Inc

Access to resources Recommend Favorite

MAVEN IUVS observations of the aftermath of the Comet Siding Spring meteor shower on Mars

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 12, 2015-06 ,pp. : 4755-4761

John Wiley & Sons Inc

Access to resources Recommend Favorite

The structure and variability of Mars upper atmosphere as seen in MAVEN/IUVS dayglow observations

GEOPHYSICAL RESEARCH LETTERS, Vol. 42, Iss. 21, 2015-11 ,pp. : 9023-9030

John Wiley & Sons Inc

Access to resources Recommend Favorite